在银河系光环中发现大规模的X射线气泡
P Predehl1, R A Sunyaev2,3, W Becker4,5
1Max-Planck-Institut für Extraterrestrische Physik, Garching, Germany. predehl@mpe.mpg.de.
Nature
|December 10, 2020
概括
发现的巨大的X射线泡距离银河系14千帕塞克
科学领域:
- * 天体物理学
- * 星系的形成和演变
- *等离子体物理
背景情况:
- *银河系的光环中含有冲击热气体, 这对于理解星系形成模型至关重要.
- * 证据表明过去的核活动将能量注入光环,但它的起源 (恒星形成与超大质量黑洞) 和与大规模特征的联系仍然不清楚.
研究的目的:
- * 为了研究能量注入银河系光环的起源和性质.
- * 确定核活动与大规模星系结构之间的因果关系.
- 描述新发现的X射线发射泡及其对环银河系介质的影响.
主要方法:
- *软X射线观测以检测和绘制泡结构.
- *分析泡边界以确定冲击特征.
- *与现有的马射线数据和星系形成的理论模型进行比较.
主要成果:
- * 发现软X射线发射泡延伸~14千帕塞克以上和以下银河系中心.
- 在南方的天空中发现一个类似北极的结构.
- * 尖的气泡边界表明无碰撞,非辐射冲击,表明星系规模结构,而不是局部超新星残留物.
结论:
- 这些X射线泡很可能是来自银河系中心的巨大能量注入造成的,
- * 估计X射线气泡的能量 (~10^56 erg) 足以显著影响环银河系介质的结构,能量和化学丰富.
- 这一发现提供了强有力的证据, 证明银河系核活动与银河系周围环境之间存在联系.
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